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dc.contributor.authorKostensalo, Joel
dc.contributor.authorSuhonen, Jouni
dc.contributor.authorZuber, K.
dc.date.accessioned2020-03-10T12:51:45Z
dc.date.available2020-03-10T12:51:45Z
dc.date.issued2020
dc.identifier.citationKostensalo, J., Suhonen, J., & Zuber, K. (2020). Calculated solar-neutrino capture rate for a radiochemical 205Tl-based solar-neutrino detector. <i>Physical Review C</i>, <i>101</i>(3), Article 031302(R). <a href="https://doi.org/10.1103/PhysRevC.101.031302" target="_blank">https://doi.org/10.1103/PhysRevC.101.031302</a>
dc.identifier.otherCONVID_34932685
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/68117
dc.description.abstractRadiochemical experiments for low-energy solar-neutrino detection have been making headlines by exploiting the isotopes 37Cl and 71Ga. Such a very low-threshold measurement of this type can also be performed using 205Tl, which has been considered for decades for this purpose. A unique feature of this detector nucleus is the integration in the solar-neutrino flux over 106 of years owing to its long-living daughter 205Pb. In this Rapid Communication, we have calculated for the first time the cross section for the charged-current solar-neutrino scattering off 205Tl. Taking into account the solar-model-predicted neutrino fluxes and the electron-neutrino survival probabilities, a solar-neutrino capture rate of 62.2 ± 8.6 solar-neutrio units is determined, a value significantly smaller than in previous estimates.en
dc.format.mimetypeapplication/pdf
dc.languageeng
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review C
dc.rightsIn Copyright
dc.subject.otherelectroweak interactions in nuclear physics
dc.subject.othernuclear structure and decays
dc.subject.othernucleus-neutrino interactions
dc.subject.othersolar neutrinos
dc.titleCalculated solar-neutrino capture rate for a radiochemical 205Tl-based solar-neutrino detector
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202003102355
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn2469-9985
dc.relation.numberinseries3
dc.relation.volume101
dc.type.versionpublishedVersion
dc.rights.copyright©2020 American Physical Society
dc.rights.accesslevelopenAccessfi
dc.relation.grantnumber318043
dc.subject.ysoydinfysiikka
dc.subject.ysohiukkasfysiikka
dc.subject.ysoneutriinot
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
jyx.subject.urihttp://www.yso.fi/onto/yso/p15576
jyx.subject.urihttp://www.yso.fi/onto/yso/p5219
dc.rights.urlhttp://rightsstatements.org/page/InC/1.0/?language=en
dc.relation.doi10.1103/PhysRevC.101.031302
dc.relation.funderResearch Council of Finlanden
dc.relation.funderSuomen Akatemiafi
jyx.fundingprogramAcademy Project, AoFen
jyx.fundingprogramAkatemiahanke, SAfi
jyx.fundinginformationThis work has been partially supported by the Academy of Finland under Academy Project No. 318043. J.K. acknowledges financial support from the Jenny and Antti Wihuri Foundation.
dc.type.okmA1


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